Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-13T02:48:26.631Z Has data issue: false hasContentIssue false
  • English
  • Français

An artificial Kepler dichotomy? Implications for the coplanarity of planetary systems

Published online by Cambridge University Press:  27 October 2016

Timothy Bovaird  and
Charles H. Lineweaver
Timothy Bovaird
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia
Charles H. Lineweaver
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia Research School of Earth Sciences, Australian National University
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We challenge the assumptions present in previous efforts to model the ensemble of detected Kepler systems, which require a dichotomous stellar population of ‘fertile’ and ‘sterile’ planet producing stars. We remove the assumption of Rayleigh distributed mutual inclinations between planets and show that the need for two distinct stellar populations disappears when the inner part of planetary disks are assumed to be flat, rather than flared.

Keywords

Keplermultiple-planet systemscoplanarityprotoplanetary disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , pp. 196
Copyright
Copyright © International Astronomical Union 2016 

References

Lissauer, J. J. et al. 2011, ApJS, 197, 8 CrossRefGoogle Scholar
Johansen, A., Davies, M. B., Church, R. P., & Holmelin, V. 2012, ApJ, 758, 39 CrossRefGoogle Scholar
Ballard, S. & Johnson, J. A. 2014, ApJ, submittedGoogle Scholar
Chatterjee, S., & Tan, J. C., 2014, ApJ 780, 53 Google Scholar